Spectral Characteristics of Large-Scale Radio Emission Areas in Coronal Holes
| Autor: | I. Yu. Grigor’eva, A. A. Kochanov, D. V. Prosovetsky |
|---|---|
| Rok vydání: | 2013 |
| Předmět: |
Physics
Range (particle radiation) Spectral index Astrophysics::High Energy Astrophysical Phenomena Coronal hole FOS: Physical sciences Scale (descriptive set theory) Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Solar atmosphere Spectral line Radio spectrum Geophysics Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science QUIET Physics::Space Physics Astrophysics::Solar and Stellar Astrophysics Astrophysics::Galaxy Astrophysics Solar and Stellar Astrophysics (astro-ph.SR) |
| DOI: | 10.48550/arxiv.1312.3718 |
| Popis: | The spectra of the coronal hole radio emission in solar cycles 23 and 24 have been studied based on RATAN-600 data in the 4-16.5 GHz range at frequencies of 5.7 and 17 GHz and 327 MHz. It has been found that bright features of coronal hole microwave emission at 17 GHz and dark features at 5.7 GHz can exist in coronal holes when the spectral index is 1.25-1.5 in the 6.5-16.5 GHz range; the radio spectrum in this range is flat when coronal holes are indiscernible against the background of a quiet Sun. The possible vertical scale of the solar atmosphere over coronal holes is discussed. Comment: 5 pages, 4 figures |
| Databáze: | OpenAIRE |
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